In the local Universe, galaxies can be divided into
two distinct populations: quiescent and star-forming
galaxies [1]}, [2]}, [3]}, [4]}.
The number density of quiescent galaxies continuously
increases with cosmic time since redshift of
about four [5]}, [6]}, [7]}, [8]}, [9]},
suggesting that galaxy quenching is an important process
that drives galaxy evolution over most of the Hubble time.
To understand the underlying mechanisms, extensive studies
have been carried out to search for the correlation of
galaxy quenching with both internal properties of galaxies and their environments
[10]}, [11]}, [12]}, [13]}, [4]}, [15]}, [16]}, [17]}, [18]}, [19]}, [20]}, [21]}.
